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Answer :
The mechanism by which solar energy reaches the Sun's photosphere from the layer just underneath it is convection.
Convection is the process by which hot material rises and cooler material sinks, creating a circulation pattern that transports energy from the Sun's interior to its surface. In this case, hot plasma in the layer just underneath the photosphere rises, carrying energy with it, and eventually reaches the photosphere where it radiates out into space as visible light and other forms of electromagnetic radiation.
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